A model of radiating black hole in noncommutative geometry

Details A model of radiating black hole in noncommutative geometry A model of radiating black hole in noncommutative geometry

2005-07-27

arxiv.org/abs/hep-th/0507266v1

J.Phys.A38:L631-L638,2005

Physics

High Energy Physics

High Energy Physics - Theory

10 pages, 4 figures

Scientific paper

10.1088/0305-4470/38/39/L02

The phenomenology of a radiating Schwarzschild black hole is analyzed in a noncommutative spacetime. It is shown that noncommutativity does not depend on the intensity of the curvature. Thus we legitimately introduce noncommutativity in the weak field limit by a coordinate coherent state approach. The new interesting results are the following: i) the existence of a minimal non-zero mass to which black hole can shrink; ii) a finite maximum temperature that the black hole can reach before cooling down to absolute zero; iii) the absence of any curvature singularity. The proposed scenario offers a possible solution to conventional difficulties when describing terminal phase of black hole evaporation.

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